Impact factor of Chinese Physics C is 3.6 in 2023 Impact factor of Chinese Physics C is 3.6 in 2022 2021 Impact Factor 2.944
Advanced Search
×
近期发现有不法分子冒充我刊与作者联系，借此进行欺诈等不法行为，请广大作者加以鉴别，如遇诈骗行为，请第一时间与我刊编辑部联系确认（《中国物理C》（英文）编辑部电话：010-88235947,010-88236950），并作报警处理。
本刊再次郑重声明：
（1）本刊官方网址为cpc.ihep.ac.cn和https://iopscience.iop.org/journal/1674-1137
（2）本刊采编系统作者中心是投稿的唯一路径，该系统为ScholarOne远程稿件采编系统，仅在本刊投稿网网址（https://mc03.manuscriptcentral.com/cpc）设有登录入口。本刊不接受其他方式的投稿，如打印稿投稿、E-mail信箱投稿等，若以此种方式接收投稿均为假冒。
（3）所有投稿均需经过严格的同行评议、编辑加工后方可发表，本刊不存在所谓的“编辑部内部征稿”。如果有人以“编辑部内部人员”名义帮助作者发稿，并收取发表费用，均为假冒。
                  
《中国物理C》（英文）编辑部
2024年10月30日
Chinese Physics C> 2017, Vol. 41> Issue(8) : 084101 DOI: 10.1088/1674-1137/41/8/084101

Ω and φ in Au+Au collisions at sqrt(SNN)=200 and 11.5 GeV from a multiphase transport model

  • 1.

     Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China

  • 2.

     University of Chinese Academy of Sciences, Beijing 100049, China

  • 3.

      Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China

  • 4.

     ShanghaiTech. University, Shanghai 200031, China

  • Within the framework of a multiphase transport model, we study the production and properties of Ω and φ in Au + Au collisions with a new set of parameters for √sNN=200 GeV and with the original set of parameters for √sNN=11.5 GeV. The AMPT model with string melting provides a reasonable description at √sNN=200 GeV, while the default AMPT model describes the data well at √sNN=11.5 GeV. This indicates that the system created at top RHIC energy is dominated by partonic interactions, while hadronic interactions become important at lower beam energy, such as √sNN=11.5 GeV. The comparison of N(Ω++Ω-)/[2N(φ)] ratio between data and calculations further supports the argument. Our calculations can generally describe the data of nuclear modification factor as well as elliptic flow.
      PCAS:
  • 加载中

  • References

    [1] Y. Aoki, G. Endrodi, Z. Fodor, S. D. Katz, and K. K. Szabo, Nature, 443:675 (2006)
    [2] F. Karsch, Prog. Theor. Phys. Suppl., 168:237 (2007)
    [3] B. I. Abelev et al (STAR Collaboration), Science, 328:58 (2010)
    [4] B. I. Abelev et al (STAR Collaboration), Nature, 473:353 (2011)
    [5] For a review paper, see eg., Yu-Gang Ma, Jin-Hui Chen, and Liang Xue, Front. Phys., 7:637 (2012)
    [6] L. Adamczyk et al (STAR Collaboration), Nature, 527:345 (2015)
    [7] Z. Q. Zhang and Y. G. Ma, Nucl. Sci. Tech., 27:152 (2016)
    [8] L. Adamczyk et al (STAR Collaboration), Phys. Rev. Lett., 112:032302 (2014)
    [9] L. Adamczyk et al (STAR Collaboration), Phys. Rev. Lett., 113:092301 (2014)
    [10] L. Adamczyk et al (STAR Collaboration), Phys. Rev. C, 92:021901(R) (2015)
    [11] C. M. Ko, F. Li, Nucl. Sci. Tech., 27:140 (2016)
    [12] For a review paper, see eg., X. F. Luo and N. Xu, Nucl. Sci. Tech., 28:in press (2017)
    [13] S. V. Afanasiev et al (NA49 Collaboration), Phys. Rev. C, 66:054902 (2002)
    [14] C. Alt et al (NA49 Collaboration), Phys. Rev. C, 77:024903 (2008)
    [15] D. E. Kharzeev, L. D. McLerran, and H. J. Warringa, Nucl. Phys. A, 803:227 (2008)
    [16] For a review paper, see eg., K. Hattori and X. Huang, Nucl. Sci. Tech., 28:26 (2017)
    [17] G. L. Ma and X. G. Huang, Phys. Rev. C, 91:054901 (2015)
    [18] L. Adamczyk et al (STAR Collaboration), Phys. Rev. Lett., 110:142301 (2013)
    [19] J. Tian, J. H. Chen, Y. G. Ma et al:Phys. Rev. C, 79:067901 (2009)
    [20] J. Xu, T. Song, C. M. Ko, and F. Li, Phys. Rev. Lett., 112:012301 (2014)
    [21] C. M. Ko et al, Nucl. Sci. Tech., 24:050525 (2013)
    [22] J. H. Chen, F. Jin, D. Gangadharan, X. Z. Cai, H. Z. Huang, and Y. G. Ma, Phys. Rev. C, 78:034907 (2008)
    [23] L. Adamczyk, et al (STAR Collaboration), Phys. Rev. C, 93:021903(R) (2016)
    [24] K. Ackermann et al. (STAR Collaboration), Nucl. Instrum. Methods A, 499:624 (2003)
    [25] Y. F. Xu, Y. J. Ye, J. H. Chen, Y. G. Ma, S. Zhang, and C. Zhong, Nucl. Sci. Tech., 27:87 (2016)
    [26] L. Ma, X. Dong, H. Qiu, S. Margetis, and Y. G. Ma, Nucl. Sci. Tech., 28:25 (2017)
    [27] Z. W. Lin, C. M. Ko, B. A. Li, B. Zhang, and S. Pal, Phys. Rev. C, 72:064901 (2005)
    [28] X. N. Wang and M. Gyulassy, Phys. Rev. D, 44:3501 (1991); M. Gyulassy and X. N. Wang, Comput. Phys. Commun., 83:307 (1994)
    [29] B. Zhang, Comput. Phys. Commum., 109:193 (1998)
    [30] B. Andersson, G. Gustafson, G. Ingelman, and T. Sjstrand, Phys. Rep., 97:31 (1983)
    [31] B. A. Li and C. M. Ko, Phys. Rev. C, 52:2037 (1995)
    [32] Z. W. Lin and C. M. Ko, Phys. Rev. C, 65:034904 (2002)
    [33] J. Xu and C. M. Ko, Phys. Rev. C, 84:014903 (2011)
    [34] Z. W. Lin, Phys. Rev. C, 90:014904 (2014)
    [35] G. L. Ma and Z. W. Lin, Phys. Rev. C, 93:054911 (2016)
    [36] B. I. Abelev et al (STAR Collaboration), Phys. Rev. C, 76:064904 (2007)
    [37] Z. W. Lin, S. Pal, C. M. Ko, B. A. Li, and B. Zhang, Phys. Rev. C, 64:011902(R) (2001)
    [38] B. I. Abelev et al (STAR Collaboration), Phys. Lett. B, 655:104 (2007)
    [39] B.I. Abelev et al (STAR Collaboration), Phys. Rev. Lett., 99:112301 (2007)
    [40] J. Adams et al (STAR Collaboration), Phys. Rev. Lett., 98:062301 (2007)
    [41] R. C. Hwa and C. B. Yang, Phys. Rev. C, 75:054904 (2007)
    [42] J. Adams et al (STAR Collaboration), Phys. Rev. Lett., 92:052302 (2004)
    [43] J. H. Chen, Y. G. Ma, and G. L. Ma et al:Phys. Rev. C, 74:064902 (2006)
    [44] For a review paper, see e.g., J. Ollitrault, Nucl. Phys. A, 638:195 (1998)
    [45] Z. W. Lin and C. M. Ko, Phys. Rev. C, 65:034904 (2002)
    [46] B. Zhang, M. Gyulassy, and C. M. Ko, Phys. Lett. B, 455:45 (1999)
    [47] D. Molnar and M. Gyulassy, Nucl. Phys. A, 697:495 (2002)
    [48] E. E. Zabrodin et al, Phys. Lett. B, 508:184 (2001)
    [49] P. F. Kolb, J. Sollfrank, and U. W. Heinz, Phys. Lett. B, 459:667 (1999); Phys. Rev. C, 62:054909 (2000)
    [50] D. Teaney, J. Lauret, and E. V. Shuryak, Phys. Rev. Lett., 86:4783 (2001)
    [51] P. Huovijnen et al, Phys. Lett. B, 503:58 (2001)
    [52] P. F. Kolb et al, Nucl. Phys., A696:197 (2001)
    [53] L. Adamczyk et al (STAR Collaboration), Phys. Rev. Lett., 116:062301 (2016)
    [54] L. Adamczyk et al (STAR Collaboration), Phys. Rev. Lett., 99:112301 (2007)
    [55] L. Adamczyk et al (STAR Collaboration), Phys. Rev. C, 93:014907 (2016)

  • Access

    加载中

Get Citation
Y. J. Ye, J. H. Chen, Y. G. Ma, S. Zhang and C. Zhong. Ω and φ in Au+Au collisions at sqrt(SNN)=200 and 11.5 GeV from a multiphase transport model[J]. Chinese Physics C, 2017, 41(8): 084101. doi: 10.1088/1674-1137/41/8/084101
Y. J. Ye, J. H. Chen, Y. G. Ma, S. Zhang and C. Zhong. Ω and φ in Au+Au collisions at sqrt(SNN)=200 and 11.5 GeV from a multiphase transport model[J]. Chinese Physics C, 2017, 41(8): 084101.  doi: 10.1088/1674-1137/41/8/084101 shu
Milestone
Received: 2017-02-03
Fund

    Supported by National Natural Science Foundation of China (11421505,11520101004,11220101005,11275250,11322547),Major State Basic Research Development Program in China (2014CB845400,2015CB856904) and Key Research Program of Frontier Sciences of CAS (QYZDJSSW-SLH002)

Article Metric

Article Views(1551)
PDF Downloads(44)
Cited by(0)
Policy on re-use
To reuse of subscription content published by CPC, the users need to request permission from CPC, unless the content was published under an Open Access license which automatically permits that type of reuse.
通讯作者: 陈斌, bchen63@163.com
  • 1. 

    沈阳化工大学材料科学与工程学院 沈阳 110142

  1. 本站搜索
  2. 百度学术搜索
  3. 万方数据库搜索
  4. CNKI搜索

Email This Article

Title:
Email:

Ω and φ in Au+Au collisions at sqrt(SNN)=200 and 11.5 GeV from a multiphase transport model

  • 1. Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China
  • 2. University of Chinese Academy of Sciences, Beijing 100049, China
  • 3.  Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China
  • 4. ShanghaiTech. University, Shanghai 200031, China
  • Received Date: 2017-02-03
  • Available Online: 2017-08-05
Fund Project:  Supported by National Natural Science Foundation of China (11421505,11520101004,11220101005,11275250,11322547),Major State Basic Research Development Program in China (2014CB845400,2015CB856904) and Key Research Program of Frontier Sciences of CAS (QYZDJSSW-SLH002)

Abstract: Within the framework of a multiphase transport model, we study the production and properties of Ω and φ in Au + Au collisions with a new set of parameters for √sNN=200 GeV and with the original set of parameters for √sNN=11.5 GeV. The AMPT model with string melting provides a reasonable description at √sNN=200 GeV, while the default AMPT model describes the data well at √sNN=11.5 GeV. This indicates that the system created at top RHIC energy is dominated by partonic interactions, while hadronic interactions become important at lower beam energy, such as √sNN=11.5 GeV. The comparison of N(Ω++Ω-)/[2N(φ)] ratio between data and calculations further supports the argument. Our calculations can generally describe the data of nuclear modification factor as well as elliptic flow.

    HTML

Reference (55)

目录

Link
IOPScience
SCOAP3
arXiv
Chinese Physical Society
Journal information
Introduction
Editorial Board
Others
Subscribe
Contact us
QQ: 1307685413
Tel: +86-010-88235947
Fax: +86-010-88233126
E-mail: cpc@ihep.ac.cn

  • CPC Website

  • IOP Website

  • CPC WeChat

Copyright © Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Beijing 100049, China 京ICP备05002789号-1

Supported by: Beijing Renhe Information Technology Co. Ltd  E-mail: info@rhhz.net

/

DownLoad:  Full-Size Img  PowerPoint
Return
Return